RPW package on Solar Orbiter
Mission Overview
Solar Orbiter is one of three candidates for the ESA's M-class mission in Cosmic Visions programme 2015-2025.Solar Orbiter aims to answer following fundamental questions in solar hand heliospheric physics
- How and where do the solar wind plasma and magnetic field originate in the corona?
- How do solar transients drive heliospheric variability?
- How do solar eruptions produce energetic particle radiation that fills the heliosphere?
- How does the solar dynamo work and drive connections between the Sun and the heliosphere?
RPW instrument package
Radio and Plasma Waves (RPW) consortium proposes a sophisticated plasma/radio wave receiver system, including high sensitivity electric and magnetic sensors. Since the receiver system covers a very wide frequency range (near-DC to 20MHz for electric, and ~0.1Hz to 500kHz for magnetic), different kinds of sensors are used for the measurements.
The package consists of following sub-systems:
- Electric antenna (ANT), consisting on a set of three monopoles and the
- Magnetic search-coil (SCM)
- BIAS unit.
- Low Frequency Receiver (LFR)
- Time Domain Sampler (TDS)
- Thermal Noise and High Frequency Receiver (TNR/HFR)
- Nominal and redundant power supply named LVPS (Low-Voltages Power Supply)
- Power Distribution Unit (PDU)
- Nominal and redundant Data Processing Unit (DPU)